December 17th, 2019
The ngVLA Project Office recently held a Town Hall on the ngVLA Project status, which is now avai...
January 31st, 2019
KSG2: Probing the Initial Conditions for Planetary Systems and Life with Astrochemistry
KSG4: Using Pulsars in the Galactic Center to Make a Fundamental Test of Gravity
KSG1: Unveiling the Formation of Solar System Analogs on Terrestrial Scales
April 24th, 2017
A fly through deep space showing the ngVLA's ability to both detect cold molecular gas, the fuel ...
January 1st, 2019
KSG3: Charting the Assembly, Structure, and Evolution of Galaxies from the First Billion Years to...
KSG5: Understanding the Formation and Evolution of Stellar and Supermassive Black Holes in the Er...
March 8th, 2018
Multi-Messenger Science & Discovery with a Next Generation Very Large Array.
January 11th, 2017
A fly through of the protoplanetary disk around HL Tau, first as seen by ALMA and the VLA, which ...
June 25th, 2020
I will discuss milliarcsecond imaging of neutron stars and accreting black holes. The exquisite ...
July 30th, 2020
Recent, remarkable images, made by the EHT collaboration of M 87, exhibit a ring of emission, pre...
July 23rd, 2020
Normally, when astronomers see beautiful, “3D” movies of the Milky Way or the stars and clouds wi...
July 2nd, 2020
The ASPECS survey is a sensitive, relatively large cosmic volume search for molecular gas across ...
July 16th, 2020
With its high sensitivity, excellent angular resolution, and wide spectral coverage, ALMA is revo...
August 6th, 2020
ALMA has revealed that planet-forming disks host a rich chemistry, with molecules displaying comp...
August 13th, 2020
The satellites of the Solar System's giant planets are one of the current frontiers of planetary ...
August 20th, 2020
Giant star clusters were an important evolutionary element of the early universe, and they appear...
August 28th, 2020
Over the past few years, we have found that small-scale "substructures" -- emission deviations on...
September 10th, 2020
Fast radio bursts (FRBs) were discovered 13 years ago. The advances in the initial phase was the ...
September 3rd, 2020
Over the past decade comprehensive and systematic studies of star formation and the gas contents ...
June 22nd, 2017
A flyover animation of the ngVLA using a notional configuration. The array contains 214 18m ante...
July 15th, 2020
NGVLA SCIENCE SYNERGIES IN THE 2030'S Eric Murphy, Robert Selina, Mark McKinnon, NRAO, United ...
THE NGVLA: REFERENCE DESIGN UPDATE Mark McKinnon, Rob Selina, Eric Murphy, NRAO/AUI, United Stat...
DEVELOPING THE NGVLA 6M RADIO TELESCOPE Gordon Lacy, Mohammad Islam, Dean Chalmers, National R...
THE NEXT GENERATION VERY LARGE ARRAY 18M ANTENNA DESIGN STUDY Dean Chalmers, Mohammad Islam, G...
FRONT END CONCEPT DEVELOPMENT FOR A NEXT GENERATION VERY LARGE ARRAY Wes Grammer, Denis Urbain...
DESIGN AND ANALYSIS OF THREE Q-BAND FEED HORNS FOR RADIO ASTRONOMY APPLICATIONS Sara Salem Hes...
DEVELOPMENT OF ORTHOMODE TRANSDUCERS (OMTS) FOR NGVLA HIGH-FREQUENCY BANDS Alvaro Gonzalez, Ke...
INTEGRATED WARM ELECTRONICS FOR THE NEXT-GENERATION VERY LARGE ARRAY Matthew Morgan, Stephen W...
STUDY OF A WIDE-AREA COHERENT/SYNCHRONOUS SYSTEM FOR NEXT GENERATION VERY LARGE ARRAY Hitoshi ...
TRIDENT FREQUENCY SLICE ARCHITECTURE CORRELATOR/BEAMFORMER REFERENCE DESIGN FOR NGVLA Michael ...
RFI MITIGATION FOR THE NGVLA : A COST-BENEFIT ANALYSIS Urvashi Rau, Rob Selina, Alan Erickson,...
December 1st, 2019
The next-generation Very Large Array promises to reshape astronomy and astrophysics. It will be a...
"INCOHERENT CLOCKING" AS A CLOCK AND TIMING SOLUTION FOR THE NGVLA? Brent Carlson, National Re...